摘要
１９９５ 至１９９８ 四年内用２ ．１６ 米望远镜、５０Ａ／ｍ ｍ 色散进行了仙后座１９９５ 新星的光谱观测。对取得的资料作了谱线证认、连续谱和谱线的流量、气壳膨胀速度、温度等测定，确定了新星气壳的电子密度和温度、估算了新星的抛射质量。指出该新星的若干特点并作了简要讨论。
The spectra of Nova Cas 1995 were observed from 1995-1998 with the 2.16m telescope at the Xinglon Station of BAO. The results of observations are described and discussed.
